Comparable energy release rates at the origin of small and large solar bursts
Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kaufmann, P. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1985 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 102(1985), 1-2 vom: Dez., Seite 97-98 |
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| Übergeordnetes Werk: |
volume:102 ; year:1985 ; number:1-2 ; month:12 ; pages:97-98 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00154040 |
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| Katalog-ID: |
OLC2033559025 |
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| 520 | |a Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates. | ||
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10.1007/BF00154040 doi (DE-627)OLC2033559025 (DE-He213)BF00154040-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kaufmann, P. verfasserin aut Comparable energy release rates at the origin of small and large solar bursts 1985 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1985 Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates. Microwave Release Rate Convolution Energy Release Repetition Rate Enthalten in Solar physics Kluwer Academic Publishers, 1967 102(1985), 1-2 vom: Dez., Seite 97-98 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:102 year:1985 number:1-2 month:12 pages:97-98 https://doi.org/10.1007/BF00154040 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 102 1985 1-2 12 97-98 |
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Comparable energy release rates at the origin of small and large solar bursts |
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Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates. © D. Reidel Publishing Company 1985 |
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Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates. © D. Reidel Publishing Company 1985 |
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Abstract The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10–100 ms suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates. © D. Reidel Publishing Company 1985 |
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